• The distance between the sun and Earth is 93,000,000 miles and the speed of light is 186,282.397 miles per second. Determine the time for light to travel from the sun to Earth. Would I set this up just like a distance problem such as Distance= rate x time? Found 2 solutions by stanbon, jim_thompson5910:
  • Minimum Distance from Sun: 741 million km (460 million miles) Surface Gravity: 23.12 m/s^2 (2.64 x Earth's) Maximum Distance from Sun: 817 million km (508 million miles) Distance across the Great Red Spot: 40,000 km (24,860 miles) Orbital Semimajor Axis: 5.20 AU (Earth=1 AU) Temperature at Cloud Tops:-150 o C (-101 o F) Minimum Distance from ...
  • On making the calculation the answer is, 16,265 statute miles. This result is only three miles greater distance than that obtained by the first process. Again in the Boston Post, for Oct. 30th, 1856, Lieut. Maury gives the following as the correct distances, in geographical miles, across the Atlantic by the various routes (circle sailing).
  • Here is what you are missing: you see the distance between the earth and the star as moving by you at 99% the speed of light. Not only do moving clocks run slow, moving lengths get shorter. The distance you see between the earth and the star is approximately 1/7 of 4.37 light years, so there are no inconsistencies.
  • Way galaxy where we live, and represented the Earth and Sun as two dots one inch apart (thus a scale of one inch equals 93 million miles—the distance between the Earth and the Sun), we would need a map at least four miles wide to locate the next nearest star, and a map 25,000 miles wide to reach the center of our galaxy.
  • Aphelion distance is 9.45 x 10 7 miles. Perihelion distance is 9.15 x 10 7 miles. Figure 2 looks rather complicated. It does, however, reveal some very important facts about the Earth and its orbit abound the sun. First note the purpleish rectangle. This represents the plane of the Earth's orbit about the sun or the Plane of the Ecliptic. We ...
When the moon is in-between the Earth and the sun, it is closer to Mars. When the Earth is in between the moon and the sun, Earth is closer to Mars. So in the end Earth and the Moon should take turns being closer, on average. $\endgroup$ – Inertial Ignorance Feb 4 '18 at 8:30
Apr 09, 2020 · If you could measure the average distance from the Earth to the Sun over the course of an entire year, you'd discover something unsettling. With each passing year that you made that measurement ...
The closest distance between Earth and the Sun is 147 million kilometers or 91 million miles, the farthest is 152 million kilometers or 94 million miles, with an average distance of 150 million kilometers or 93 million miles. The most outstanding feature of Earth is its life.Q: If the sun is disappearing into the distance, shouldn't it get smaller as it recedes? A: The sun remains the same size as it recedes into the distance due to a magnification effect caused by the intense rays of light passing through the strata of the atmolayer. From Chapter 10 of the book Earth Not a Globe we read:
The average distance between the Sun and the Earth is about 92,935,700 miles. Astronomers refer to this distance as one astronomical unit-the distance light travels in about eight and a half minutes. Earth's orbit is actually not perfectly circular; the distance between the Earth and the Sun varies slightly over the course of the year.
Explanation: So the distance between the earth and the sun is 150 million kilometers. In scientific notation, you have to find the number between 1 and 10, then multiply it by 10x. So the number between 1 and 10 in 150,000,000 is 1.5, and a number of decimal points is 8.I take it you mean 9.3 x 10^7 miles. 1 mile = 1.609 km = 1609 m. Multiply by these factors to get the conversion.
Where space begins… can actually be determined by the speed of the space vehicle and its altitude above the Earth. Consider, for instance, the record flight of Captain Iven Carl Kincheloe Jr. in an X-2 rocket plane. Kincheloe flew 2000 miles per hour (3,200 km/h) at 126,000 feet (38,500 m), or 24 miles up. By observation of parallax. Edmund Halley (of comet fame) was the first to come up with the idea to determine the Sun's distance by observing the transit of Venus.

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